Search results for "Ground"

showing 10 items of 2432 documents

Assessment of PAHs and total content of organic matter in Landfill Leachate and Groundwater

2006

PAHsmonitoring of ground watermonitoring wód podziemnychorganic carbonskładowiska odpadówwęgiel organicznydumting siteEcological Chemistry and Engineering. A
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Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube

2017

[EN] The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by ANTARES, within +/- 500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission …

POINT-LIKEGravitational-wave observatoryPhysics and Astronomy (miscellaneous)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyELECTROMAGNETIC COUNTERPARTSastro-ph.HE; astro-ph.HEAstrophysics01 natural sciences7. Clean energylocalizationIceCubeBinary black holeLIGO010303 astronomy & astrophysicsTelescopeGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEFollow-upData-acquisition systemobservatoryNeutrino detectorElectromagnetic counterpartsSIMULATIONBlack-hole mergersLigoGamma-ray burstsNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHost galaxiesSimulationGravitational waveBLACK-HOLE MERGERSAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesDATA-ACQUISITION SYSTEMGravitational wavesneutrino: productionGeneral Relativity and Quantum CosmologyBinary black holeOnes gravitacionalsLiGO Observatory0103 physical sciencesNeutrinoGW151226ddc:530NeutrinsNeutrinos010306 general physicsPoint-likeANTARESCosmologiaGravitational wavebackgroundgravitational radiationAstronomy530 PhysikLIGONeutron starGravitational Waves Neutrinos Antares IceCube LIGOAntaresPhysics and Astronomyblack hole: binary13. Climate action:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAAstronomiaDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]FOLLOW-UPPhysical Review D. Particles and Fields
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A comparison of physical activity levels in childcare contexts among Finnish and Dutch three-year-olds

2016

The aim of the current study was to determine Finnish and Dutch three-year-old preschool children's physical activity (PA) levels and how levels vary across gender, location, time of day and social contexts in both countries. A modified version of the Observational System for Recording Physical Activity in Children-Preschool (OSRAC-P) was used to measure children's PA levels and contextual variables (e.g. group composition, prompts) of children attending childcare centres in Finland and the Netherlands. In total, 90 Finnish children (46 boys and 44 girls) and 97 Dutch children (46 boys and 51 girls) were observed. Three-level linear regression analyses with cross level interactions were use…

PRESCHOOL-CHILDRENENVIRONMENTpreschool childrenPLAYGROUNDSchildcare centreSocial environmentRegression analysis030229 sport sciencesPhysical activity levelEducationLikert scaleDevelopmental psychology03 medical and health sciencesdirect observationAGE0302 clinical medicineNaturalistic observationcountry comparisonDevelopmental and Educational PsychologyObservational study030212 general & internal medicineComparative educationPsychologyLocationphysical activity (PA)European Early Childhood Education Research Journal
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The landscape of strongholds

2016

La difesa dei territori ha offerto risultati straordinari alla formazione e alla trasformazione del territorio e del paesaggio, a volte con tratti spettacolari e dimensioni incredibili. La celebrazione del centenario dell’inizio della Prima guerra mondiale ha offerto lo spunto per una riflessione sulle ricadute indotte sul paesaggio dagli eventi bellici, e più in generale dalla realizzazione di strutture difensive e del loro rapporto con il paesaggio circostante. Territorial defence led to extraordinary results in terms of forming and transforming the territory and landscape, at times with spectacular sights and incredible sizes. The one hundred year anniversary since the beginning of the F…

Paesaggio guerra trasformazioni difese muraglia canali fortezze fortificazioni canali linee d'acquaSettore ICAR/15 - Architettura Del PaesaggioLandscape strongholds waterline Great Wall Netherlands transformations land ground borders
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Identifying sedimentary structures and spatial distribution of tsunami deposits with GPR - examples from Spain and Greece

2011

Shallow drilling in coastal areas like southern Spain and different parts of Greece (Corinth region and Argolis Gulf) proved evidence for tsunamis. Sedimentary analyses were conducted to identify tsunamigenic deposits, but did not reveal sedimentary structures or spatial distribution of tsunamites in a regional scale. Since drilling is time-intensive and expensive (depending on extend), this method can by far not cover an entire coastal area. On the other hand, distribution and preservation of tsunamigenic deposits seems to be highly variable. We used ground penetrating radar (GPR) in combination with electrical resistivity tomography (ERT) measurements and sedimentological research methods…

PaleontologyBasement (geology)Ground-penetrating radarErosionDrillingSedimentSedimentary rockElectrical resistivity tomographyGeomorphologyGeologySedimentary structures2011 6th International Workshop on Advanced Ground Penetrating Radar (IWAGPR)
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Effect of dual biotic stress on plant volatile synomones used by an egg parasitoid

Plants respond to arthropod herbivory with the induction of volatiles called herbivore-induced plant volatiles (HIPVs). These volatiles appear to be important sources of information that attract parasitoids. Parasitic wasps foraging decisions are often affected by community characteristics such as community diversity and complexity. As part of a complex habitat, the presence of unsuitable hosts (non-host) may affect foraging behavior of parasitoids. In this chapter, we outline the importance of the presence of unsuitable herbivores on the behavioral responses of parasitoids. First we review the foraging behavior of parasitoid in tritrophic interaction. Then we focus on foraging behavior by …

Parasitoids. HIPVs. non-host. above- ground. below-ground [Key-words]Key-words: Parasitoids. HIPVs. non-host. above- ground. below-ground
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Potential of interactive multiobjective optimization in supporting the design of a groundwater biodenitrification process

2019

The design of water treatment plants requires simultaneous analysis of technical, economic and environmental aspects, identified by multiple conflicting objectives. We demonstrated the advantages of an interactive multiobjective optimization (MOO) method over a posteriori methods in an unexplored field, namely the design of a biological treatment plant for drinking water production, that tackles the process drawbacks, contrarily to what happens in a traditional volumetric-load-driven design procedure. Specifically, we consider a groundwater denitrification biofilter, simulated by the Activated Sludge Model modified with two-stage denitrification kinetics. Three objectives were defined (nitr…

Pareto optimalityDecision support systemdecision supportEnvironmental EngineeringProcess (engineering)Computer science0208 environmental biotechnologypäätöksentukijärjestelmät02 engineering and technologyActivated sludge model010501 environmental sciencesManagement Monitoring Policy and Law01 natural sciencesMulti-objective optimizationInteractive methodIND-NIMBUSWater treatmentSensitivity (control systems)Process engineeringWaste Management and DisposalGroundwater0105 earth and related environmental sciencesvedenpuhdistusNitratesSewagepareto optimalitypareto-tehokkuusbusiness.industrywater treatmentGeneral Medicineinteractive methodvedenkäsittelymonitavoiteoptimointi020801 environmental engineeringDecision supportRange (mathematics)Decision support; IND-NIMBUS; Interactive method; NIMBUS method; Pareto optimality; Water treatment; Algorithms; Denitrification; Nitrates; Sewage; GroundwaterDenitrificationA priori and a posterioriWater treatmentNIMBUS methodbusinessAlgorithms
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The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector

2010

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2 - 200 TeV. The result is compared to different atmospheric neutrino models and it is compatible with the atmospheric neutrinos from pion and kaon decays. No significant contribution from charm hadron decays or extraterrestrial neutrinos is detected. The capabilities to improve the measurement of the neutrino spectrum with the successor experiment IceCube are discussed.

Particle physicsAMANDA[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Solar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAMANDA; Atmospheric neutrinos; Cherenkov radiation; Neural net; Unfoldingneural netFOS: Physical sciencesAetiology screening and detection [ONCOL 5]01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsunfoldingPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cherenkov radiationHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsSolar neutrino problematmospheric neutrinosCosmic neutrino backgroundNeutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Combination of Tevatron searches for the standard model Higgs boson in the W+W- decay mode.

2010

11 páginas, 4 figuras, 1 tabla.-- CDF Collaboration: et al.

Particle physicsAstrophysics::High Energy Astrophysical PhenomenaTevatronFOS: Physical sciencesGeneral Physics and AstronomyElementary particleddc:500.2.PARTON DISTRIBUTIONS; HADRON COLLIDERS; QCD; NNLO7. Clean energy01 natural sciences114 Physical sciencesHigh Energy Physics - ExperimentStandard ModelNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle decay0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Grand Unified TheoryHADRON COLLIDERSFermilabTEVATRONNuclear Experiment010306 general physicsBosonPhysicsHIGGS BOSON010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyQCD3. Good healthPARTON DISTRIBUTIONSHiggs bosonCDFPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNNLOAnti-p p: interaction | Higgs particle: search for | gluon gluon: fusion | intermediate boson: fusion | quark antiquark: annihilation | Higgs particle: decay | Higgs particle --> W+ W- | W: pair production | W: leptonic decay | dilepton: final state | jet: multiplicity | cross section: upper limit | mass dependence | Higgs particle: mass | background | DZERO | CDF | Batavia TEVATRON Coll | anti-p p --> Higgs particle anything | anti-p p --> Higgs particle anything intermediate boson anything | anti-p p --> Higgs particle anything quark antiquark anything | 1960 GeV-cmsPhysical review letters
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Do we have any hope of detecting scattering between dark energy and baryons through cosmology?

2020

We consider the possibility that dark energy and baryons might scatter off each other. The type of interaction we consider leads to a pure momentum exchange, and does not affect the background evolution of the expansion history. We parametrize this interaction in an effective way at the level of Boltzmann equations. We compute the effect of dark energy-baryon scattering on cosmological observables, focusing on the Cosmic Microwave Background (CMB) temperature anisotropy power spectrum and the matter power spectrum. Surprisingly, we find that even huge dark energy-baryon cross-sections $\sigma_{xb} \sim {\cal O}({\rm b})$, which are generically excluded by non-cosmological probes such as col…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)cosmic background radiationAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesCosmologyGeneral Relativity and Quantum Cosmologycosmic background radiation cosmological parameters cosmology observations dark energy large-scale structure of UniverseHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencescosmological parametersdark energy010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsEquation of state (cosmology)Matter power spectrumSpectral densityAstronomy and AstrophysicsCosmic varianceHigh Energy Physics - Phenomenologyobservations13. Climate actionSpace and Planetary ScienceDark energylarge-scale structure of UniversecosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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